Astronomy Notes / Life cycle of stars
Astronomy Notes / Life cycle of stars
Astronomy Notes / Life cycle of stars
LIFE CYCLE OF STARS
·
Proto
Star
Formed
by compression of galactic gas and dust which causes Nuclear Fusion, emitting
large amount of heat and light
·
Red
Giants
Continued
Nuclear Fusion over a period of time result in depletion of hydrogen and the
helium core becomes increasingly heavy, resulting into swelling and reddening
of outer regions
Stars
of gigantic dimensions are termed as Red Giants
·
Novae
& Supernovae
Stars
whose brightness increase suddenly by ten to twenty magnitudes or more due to
partial or outright explosion in the star
When
brightness increases to 20 magnitudes or more - supernovae
·
White
Dwarfs
A
novae or Supernovae explosion in a star like our Sun may leave behind a very
dense core of that star
A
star of this size cools and contracts to become a White Dwarf
·
Neutron
Star
A
Supernovae explosion in a star bigger than the Sun may leave behind an
extremely dense, residual core of that star
·
Pulsar
The
extremely dense core left after the explosion of a bigger star: neutron star
Because
of their small size, neutron stars spin very fast and while spinning, radiate
all kinds of electro-magnetic radiations – Pulsar
Jocelyn
Bell discovered the first pulsar in 1967
·
Black
Holes
Stars
having mass greater than three times that of the sun, have contracted so much
because of their great gravitational power and have developed super density
It
is so dense that nothing, not even light can escape from its gravity and hence
called Black hole
·
Fixed
stars
Stars
which do not appear to alter their relative positions in the sky. They are
called dog stars
·
Binary
stars
Group
of two stars revolving round each other under mutual gravitational attraction
·
Temporary
stars
Those
who suddenly flare up to a greatly increased brightness and fade away after a
short time. They are called novae
·
Variable
stars
Stars
are brightness of which varies from time to time
Astronomy Notes / Life cycle of stars

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